The interaction of galaxies with their environment is a crucial issue to understand their formation and evolution. A huge effort has been devoted, from...
Understanding the Milky Way galaxy - prospects from on-going and future surveys
Galactic Archeology is today a vibrant field of research. The adoption and launch of the Gaia astrometric satellite by ESA has resulted in many spectroscopic...
Understanding the obscuring torus and the nuclear star formation of AGN using GTC/CanariCam observations
The fueling of black holes occurring in active galactic nuclei (AGN) is fundamental to the evolution of galaxies. AGN themselves are largely explained in the...
Unveiling the (optical) low surface brightness Universe: The Intracluster Light
There is a huge amount of astrophysical events that remain barely studied due to the lack of large, multiwavelength and deep optical surveys. This is the...
Unveiling the inner Milky Way globular cluster system
A serious limitation in the study of the Galactic inner halo and bulge globular clusters has been the existence of large and differential extinction by...
Using big data to understand galaxies in our neighborhood
How galaxies form and evolve remains one of the cornerstone questions in our understanding of the universe on grand scales. While much progress has been made by...
Using nitrogen as a tracer of the chemical content of the Universe: from WR nebulae to early star-forming galaxies
Chemical abundances derived using emission-line spectra in ionized gaseous nebulae are between the most useful properties that can be derived to understand the...
Warps of disk galaxies are ubiquitous. In almost every disk galaxy a bending of the disk occurs where the stars fade away and hence where the dark matter halo...
WEAVE: The next generation wide-field spectroscopy facility for the WHT
I will describe the major scientific motivation and outline design concept for a new 2 degree field, 1000 fibre multi-object spectroscopy facility for the WHT...